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Zero sound and higher-form symmetries in compressible holographic phases

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arxiv 2210.14802 v2 pith:SJDC5MWP submitted 2022-10-26 hep-th cond-mat.str-el

Zero sound and higher-form symmetries in compressible holographic phases

classification hep-th cond-mat.str-el
keywords symmetrymodezeroholographicstatesemergentglobalhigher-form
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Certain holographic states of matter with a global U(1) symmetry support a sound mode at zero temperature, caused neither by spontaneous symmetry breaking of the global U(1) nor by the emergence of a Fermi surface in the infrared. In this work, we show that such a mode is also found in zero density holographic quantum critical states. We demonstrate that in these states, the appearance of a zero temperature sound mode is the consequence of a mixed `t Hooft anomaly between the global U(1) symmetry and an emergent higher-form symmetry. At non-zero temperatures, the presence of a black hole horizon weakly breaks the emergent symmetry and gaps the collective mode, giving rise to a sharp Drude-like peak in the electric conductivity. A similar gapped mode arises at low temperatures for non-zero densities when the state has an emergent Lorentz symmetry, also originating from an approximate anomalous higher-form symmetry. However, in this case the collective excitation does not survive at zero temperature where, instead, it dissolves into a branch cut due to strong backreaction from the infrared, critical degrees of freedom. We comment on the relation between our results and the application of the Luttinger theorem to compressible holographic states of matter.

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